Radio Pulse Properties of the Millisecond Pulsar PSR J0437-4715
F. A. Jenet +4 more
openalex +2 more sources
Galaxy radio pulsar population modelling and magellanic clouds radio pulsar survey
published_or_final_version ; Physics ; Doctoral ; Doctor of ...
openaire +2 more sources
Millisecond Pulsars in M2: New Discoveries and a Detailed Timing Analysis
Globular clusters (GCs) offer a unique environment for discovering and studying millisecond pulsars. In this paper, we present a multiepoch search and detailed timing analysis of millisecond pulsars in the GC M2, using the Five-hundred-meter Aperture ...
Baoda Li +15 more
doaj +1 more source
The radio spectrum of micropulses from pulsar PSR 0950 + 08
B. J. Rickett +2 more
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Upper limits on gravitational wave emission from 78 radio pulsars [PDF]
B. Abbott +99 more
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White Noises on Different Stokes Components of Six Millisecond Pulsars
We presented measurements of jitter noise and radiometer noise for the Stokes parameters I , L , and V in six millisecond pulsars from the International Pulsar Timing Array sample, based on FAST observations.
S. N. Sun, N. Wang, W. M. Yan
doaj +1 more source
DISCOVERY OF TWO MILLISECOND PULSARS INFERMISOURCES WITH THE NANÇAY RADIO TELESCOPE [PDF]
I. Cognard +31 more
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Einstein@Home Searches for Gamma-Ray Pulsars in the Inner Galaxy
The Fermi Large Area Telescope (LAT) has revealed a mysterious extended excess of GeV gamma-ray emission around the Galactic Center (GC), which can potentially be explained by unresolved emission from a population of pulsars, particularly millisecond ...
C. J. Clark +16 more
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A Radio Frequency Study of the Accreting Millisecond X-ray Pulsar, IGR J16597–3704, in the Globular Cluster NGC 6256 [PDF]
Alexandra J. Tetarenko +16 more
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Radio Emission across the Entire Rotation Phases of Pulsars
Supersensitive observations of bright pulsars by the Five-hundred-meter Aperture Spherical Telescope have revealed weak radio emission continuously emerges in the rotation phases between the “main” pulse and “interpulse” of a rotating neutron star.
P. F. Wang, J. L. Han
doaj +1 more source

